challenges in seafloor imaging and mapping with synthetic aperture sonar

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Challenges in Seafloor Imaging and Mapping with Synthetic Aperture Sonar Roy E Hansen, Hayden J Callow, Torstein O Sæbø and Stig A V Synnes Norwegian Defence Research Establishment (FFI) P O Box 25, NO-2027 Kjeller, Norway Abstract The success of synthetic aperture sonar (SAS) is critically dependent on overcoming several challenges. The sonar has to be positioned with accuracy better than a fraction of a wavelength along the synthetic aperture. The ocean environment, and particularly the sound velocity, has to be accurately estimated for successful focusing of SAS images. For non- straight synthetic apertures, the bathymetry of the scene to be imaged must be known. Kongsberg Maritime and FFI have developed the HISAS 1030 wideband widebeam interferometric SAS. This paper describes the system and show example results from data collected by a HUGIN 1000-MR autonomous underwater vehicle. 1 Introduction Synthetic aperture sonar (SAS) is less known and devel- oped than its counterpart in radar. Although the princi- ple of SAS is not new [1], it is only during latest years that SAS systems have become commercially available. The Norwegian Defence Research Establishment (FFI) and Kongsberg Maritime have a long term collaboration to develop SAS for the HUGIN autonomous underwater vehicle (AUV). Figure 1 shows a HUGIN 1000-MR AUV onboard a Royal Norwegian Navy mine hunter. There are a few critical differences between SAR and SAS – one in particular is the environment for which the sensor is oper- ating. This paper describes some of the specific challenges in SAS and how we approach them in imaging and map- ping of the seafloor from autonomous underwater vehicles (AUVs). Figure 1: HUGIN 1000-MR AUV onboard the Royal Nor- wegian Navy mine hunter Hinnøy. 2 System description Figure 2: The HISAS 1030 interferometric SAS. HISAS 1030 is a wideband widebeam interferometric SAS developed by Kongsberg Maritime and FFI [2]. The sonar contains two along-track receiver arrays of length 1.2 m with 32 elements in each array, and a vertical baseline of 20 wavelengths. The transmitter is a vertical phased ar- ray with reception capability. Figure 2 shows the sonar mounted on a HUGIN vehicle. Typical HISAS 1030 spec- ifications are summarized in Table 1. Center frequency [kHz] 100 Wavelength [cm] 1.5 Typical bandwidth [kHz] 30 Total frequency range [kHz] 50-120 Along-track resolution [cm] 3 Cross-track resolution [cm] 3 Maximum range @ 2 m/s [m] 200 Area coverage rate km 2 /h 2 Table 1: Typical system specifications.

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Challenges in Seafloor Imaging and Mapping with Synthetic Aperture Sonar Roy E Hansen, Hayden J Callow, Torstein O Sæbø and Stig A V Synnes Norwegian Defence Research Establishment (FFI) P O Box 25, NO-2027 Kjeller, Norway
Abstract
The success of synthetic aperture sonar (SAS) is critically dependent on overcoming several challenges. The sonar has to be positioned with accuracy better than a fraction of a wavelength along the synthetic aperture. The ocean environment, and particularly the sound velocity, has to be accurately estimated for successful focusing of SAS images. For non- straight synthetic apertures, the bathymetry of the scene to be imaged must be known. Kongsberg Maritime and FFI have developed the HISAS 1030 wideband widebeam interferometric SAS. This paper describes the system and show example results from data collected by a HUGIN 1000-MR autonomous underwater vehicle.
1 Introduction Synthetic aperture sonar (SAS) is less known and devel- oped than its counterpart in radar. Although the princi- ple of SAS is not new [1], it is only during latest years that SAS systems have become commercially available. The Norwegian Defence Research Establishment (FFI) and Kongsberg Maritime have a long term collaboration to develop SAS for the HUGIN autonomous underwater vehicle (AUV). Figure 1 shows a HUGIN 1000-MR AUV onboard a Royal Norwegian Navy mine hunter. There are a few critical differences between SAR and SAS – one in particular is the environment for which the sensor is oper- ating. This paper describes some of the specific challenges in SAS and how we approach them in imaging and map- ping of the seafloor from autonomous underwater vehicles (AUVs).
Figure 1: HUGIN 1000-MR AUV onboard the Royal Nor- wegian Navy mine hunter Hinnøy.
2 System description
Figure 2: The HISAS 1030 interferometric SAS.
HISAS 1030 is a wideband widebeam interferometric SAS developed by Kongsberg Maritime and FFI [2]. The sonar contains two along-track receiver arrays of length 1.2 m with 32 elements in each array, and a vertical baseline of 20 wavelengths. The transmitter is a vertical phased ar- ray with reception capability. Figure 2 shows the sonar mounted on a HUGIN vehicle. Typical HISAS 1030 spec- ifications are summarized in Table 1.
Center frequency [kHz] 100 Wavelength [cm] 1.5 Typical bandwidth [kHz] 30 Total frequency range [kHz] 50-120 Along-track resolution [cm] 3 Cross-track resolution [cm] 3 Maximum range @ 2 m/s [m] 200 Area coverage rate km2/h 2
Table 1: Typical system specifications.
sas
EUSAR 2010
Figure 3 shows an example image that captures the essence of SAS and illustrates the performance of HISAS 1030.
Figure 3: Example image that illustrates the performance of HISAS 1030. The range is 25–325 m (left to right) and the water depth 180–200 m. Top inset: A 40×20 m cutout around the wreck of the German WW2 submarine U-735, centred at 225 m range. Bottom insets: Cutout around 1×1 m concrete cubes, centred at 275 m range (left) and 320 m range (right). Theoretical resolution in the image is 3 × 3 cm.
3 Differences between SAR and SAS
The principle for synthetic aperture imaging is the same in radar and sonar. There are, however, some rather impor- tant differences between SAR and SAS. These differences are related to the ocean environment and the differences in phase velocity.
3.1 Frequency Seawater is a dissipative medium through viscosity and chemical processes [3]. Acoustic absorption in seawater is frequency dependent, such that the travelling distance measured in wavelengths has a fixed absorption loss (see Table 2). This gives an upper limit on the frequency for any given range. This will, inherently, limit the cross-range resolution for real aperture sonars, such as sidescan sonar and multibeam echosounders [3].
f [kHz] R [km] λ [m] 0.1 1000 15 1 100 1.5 10 10 0.15 100 1 0.015 1000 0.1 0.0015
Table 2: Approximate range R for frequency f and corre- sponding wavelength λ.
3.2 Along-track sampling The most significant difference between SAR and SAS is the phase velocity, which typically is cr = 3× 108 m/s for radio waves in air, and ca = 1.5 × 103 m/s for acoustic waves in seawater. The low phase velocity causes a fun- damental problem in obeying the sampling criterion along the synthetic array. Using a multi-element receiver array is a simple way to overcome this problem [1, 4], and almost all existing SAS systems today are designed with multi- element receivers. The distance travelled between pulses can maximally be half the lenghth of the receiver array [4]. This gives a maximum range of
Rmax = cL
4αv
where c is the sound velocity, L is the physical receiver array length, v is the vehicle speed, and α is an over- lap factor ≥ 1 controlling the relative redundancy in the synthetic aperture. This redundancy is used for micron- avigation (see section 4.1). As an example, the HISAS 1030 has L = 1.2 m. This gives a maximum range of Rmax = 203 m at vehicle speed v = 2 m/s and overlap factor α = 32/29.
3.3 Imaging geometry A typical SAS imaging geometry is illustrated in Figure 4. Two sonars are mounted on the vehicle, one on port side and one on starboard. The vehicle runs rather low over the seafloor, and the sonar range is typically 10 times the vehi- cle altitude. Beneath the vehicle, there is a blind zone or a gap with a width approximately two times the altitude. The imaging geometry is thereby rather horizontal with recep- tion of data from 45 to 5 grazing angle. The SAS system works solely in strip-map mode, and the swath width is al- most equal to the maximum range. Shadowing is a more
important effect than foreshortening and layover compared to satellite borne SAR.
Figure 4: AUV based SAS imaging geometry
4 Challenges in SAS The success of synthetic aperture sonar (SAS) is critically dependent on overcoming several challenges [5, 6]. In this section, we list some of the important factors to consider to be able to perform robust and reliable SAS.
4.1 Navigation Navigation of autonomous underwater vehicles has differ- ent challenges than e.g. airborne platforms since GPS is not available. The HUGIN AUV is equipped with a high grade aided inertial navigation system (INS). In SAS, the sonar has to be positioned with accuracy better than a frac- tion of a wavelength along the entire synthetic aperture. At 100 kHz this equals an accuracy requirement around 1 mil- limetre along tens of metres of travelled distance. This re- quirement is generally not met even by the most advanced aided INSes available for AUVs. We solve this by integrat- ing micronavigation on sensor data with the inertial navi- gation [7]. The micronavigation is based on the principle of displaced phase centre antenna (DPCA) [8]. In radar, DPCA is mostly used for clutter supression in ground mov- ing target indication (GMTI) radar. We use DPCA to esti- mate platform motion (similar to shear averaging in SAR).
4.2 Sound velocity errors The sound velocity in the ocean varies with depth [3]. In coastal waters, there might also be local horizontal and temporal variations. These variations can cause variation in the sound velocity up to 2% along the acoustic path. SAS is near-field acoustic imaging, which requires that the geometry and the sound velocity between observation sys- tem (sonar) and scene (seafloor) to be known. An incor- rect sound velocity leads to defocusing and reduced image quality [9]. We approach the problem of estimating sound velocity in several ways. First, the vehicle carries a high quality Con- ductivity, Temperature, Depth (CTD) sensor from which the in-situ sound velocity is calculated [3]. All the CTD data are used to create the best possible CTD map for the SAS processing. For residual errors in the sound velocity causing defocusing in the SAS imagery, we have devel- oped a blind image correction technique that both corrects
the image and estimates the error in the average sound ve- locity [9]. This technique is based on phase gradient auto- focusing [10].
4.3 Bathymetry
Figure 5: Vehicle track and seafloor depth for a particular HUGIN AUV mission in Norwegian waters.
For non-straight synthetic apertures, the topography (or bathymetry) of the scene to be imaged has to be known [10]. This is critical for robust autonomous underwater ve- hicle (AUV) based SAS in areas with rough terrain. Fig- ure 5 shows the vehicle depth and seafloor depth for a par- ticular HUGIN AUV track in rough terrain. The two indi- cated sections are time slots for data collection for different SAS imaging blocks. The vertical motion is clearly non- straight, and the topography has to be estimated. We ap- proach this by applying real aperture interferometric map- ping of the swath as part of the preprocessing before syn- thetic aperture imaging [6].
4.4 Shallow waters
Figure 6: Interferometric SAS in shallow waters
A fundamental challenge in high resolution imaging of the seafloor is surveying in shallow waters, where the presence of the sea surface affects the imaging quality. This applies both to real aperture sonar (also known as sidescan sonar [3]), and SAS. Figure 6 shows the basic geometry for di- rect signals and multipath (or clutter) signals that has been reflected one or more times in the surface. Multipath will affect SAS threefold: 1) the image signal to clutter ratio will be lower; 2) the spatial coherence between the upper and the lower receiver array will decrease [11]; 3) the tem- poral coherence between pings (used in the principle of DPCA [8]) will be lower. This is strongly dependent on the ocean environment.
Figure 7: The effect of multipath in shallow waters. The range (x-axis) is 150 m and the water depth is only 9 m.
Figure 7 shows two SAS images of the same area of the seafloor, taken one week apart. The wind speed was rela- tively high during the data collection for the upper image, while during the data catch for the lower image, the sea was calm. This caused sufficient difference in sea surface roughness, to change the multipath contribution. We use the spatial coherence from the real aperture interferometer to calculate an equivalent signal to clutter ratio [12, 11]. The red curve in the lower image indicates the range for which the coherence is 0.66. We use this to mark the valid range in shallow water operations.
5 Summary
There are significant differences between SAR and SAS, all related to the ocean environment. HISAS 1030 is a wideband widebeam interferometric SAS developed by Kongsberg Maritime and FFI. In this paper, we have listed some of the specific challenges that has to be solved to ob- tain robustness and high performance. These actions affect both the design of the sonar, the signal processing of the sonar data and the control of the platform. We combine sonar micronavigation with aided inertial navigation to ob- tain sufficient navigation accuracy. We map the terrain us- ing real aperture interferometry as part of the SAS process- ing such that reliable imagery can be performed in rough terrain. We estimate sound velocity errors and correct for it in the SAS images. In shallow waters, we estimate the range for validity by inspecting the spatial coherence func- tion.
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